
Cosmic Microwave Background (CMB) Observations: We consider the measurements of the CMB observations from the final release of the Planck 2018 team. In particular, we have used the CMB temperature and polarization power spectra, that means
plikTTTEEE+lowl+lowE from Planck 2018 [1]}, [2]}.

Baryon Acoustic Oscillations (BAO): Various measurements of the BAO data have been used in this work. In particular we have used the measurements from
6dFGS [3]}, SDSS-MGS [4]}, and
BOSS DR12 [5]} as considered by the Planck 2018 team [1]}.

Pantheon sample from Supernovae Type Ia (SNIa): Along with the CMB and BAO measurements, another potential cosmological probe is the SNIa, the fist observational data indicating the accelerating expansion of the Universe. Here we took a recent collection of SNIa, known as the Pantheon sample [7]} distributed in the redshift interval \(z \in [0.01, 2.3]\) .

